The relativistic equations of stellar structure and evolution. Stars with degenerate neutron cores. 1: Structure of equilibrium models

Details The relativistic equations of stellar structure and evolution. Stars with degenerate neutron cores. 1: Structure of equilibrium models The relativistic equations of stellar structure and evolution. Stars with degenerate neutron cores. 1: Structure of equilibrium models

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976stin...7627134t&link_type=abstract

Unknown

Statistics

Applications

Relativistic Theory, Stellar Evolution, Stellar Structure, Applications Of Mathematics, Energy Distribution, Mass Distribution, Newton Theory, Radii

Scientific paper

The general relativistic equations of stellar structure and evolution are reformulated in a notation which makes easy contact with Newtonian theory. Also, a general relativistic version of the mixing-length formalism for convection is presented. Finally, it is argued that in previous work on spherical systems general relativity theorists have identified the wrong quantity as "total mass-energy inside radius r."

Affiliated with

Also associated with

No associations

Rating

The relativistic equations of stellar structure and evolution. Stars with degenerate neutron cores. 1: Structure of equilibrium models does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The relativistic equations of stellar structure and evolution. Stars with degenerate neutron cores. 1: Structure of equilibrium models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The relativistic equations of stellar structure and evolution. Stars with degenerate neutron cores. 1: Structure of equilibrium models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1798351